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M. L. Hamadouche

Identifiers

  • name variant M. L. Hamadouche 0.60 · backfill

Papers (14)

  1. JWST PRIMER: strong evidence for the environmental quenching of low-mass galaxies out to $\mathbf{\textit{z} \simeq 2}$ astro-ph.GA · 2024 · author #1
  2. The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5 astro-ph.GA · 2024 · author #16
  3. The NIRVANDELS Survey: the stellar and gas-phase mass-metallicity relations of star-forming galaxies at z = 3.5 astro-ph.GA · 2024 · author #14
  4. JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$ astro-ph.GA · 2024 · author #16
  5. The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10 astro-ph.GA · 2023 · author #13
  6. The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue astro-ph.GA · 2023 · author #32
  7. Connecting the escape fraction of Lyman-alpha and Lyman-continuum photons in star-forming galaxies at $\mathbf{z\simeq 4-5}$ astro-ph.GA · 2023 · author #9
  8. A massive quiescent galaxy at redshift 4.658 astro-ph.GA · 2023 · author #11
  9. The ultraviolet continuum slopes ($\mathbf{\beta}$) of galaxies at $\mathbf{z\simeq8-16}$ from JWST and ground-based near-infrared imaging astro-ph.GA · 2022 · author #9
  10. A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS astro-ph.GA · 2022 · author #8
  11. The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging astro-ph.GA · 2022 · author #8
  12. A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses and star-formation histories astro-ph.GA · 2022 · author #4
  13. The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5 astro-ph.GA · 2022 · author #7
  14. A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\mathbf{\textit{z} = 0.6}$ to $\mathbf{\textit{z} = 1.3}$ astro-ph.GA · 2022 · author #1

Mentions

  • 2412.09592 #1 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2405.02242 #16 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2403.03171 #16 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2405.00774 #14 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2311.06209 #13 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2306.03916 #9 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2309.14436 #32 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2301.11413 #11 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2208.00986 #8 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2208.04914 #9 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2207.12356 #8 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2207.08778 #4 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2202.04088 #7 · arxiv_oai · confidence 0.70 M. L. Hamadouche
  • 2201.10576 #1 · arxiv_oai · confidence 0.70 M. L. Hamadouche

Frequent Coauthors